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Fig. 1.
Supergiant shell SMC-SGS1 in the Wing of the SMC. The H II regions (N 88,89, and 90), clusters (NGC 602 and NGC 602c), and the supernova remnant (SNR) in the region are indicated on the color composite (Hα, [O III]) image, taken from the Magellanic Cloud Emission-Line Survey (MCELS, Winkler et al. 2005).
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